太周探测:从60年代四大天文发现说起(下)  

Teracycle Detection:Starting from the Four Major Astronomical Discoveries in 1960s(Ⅱ)

作　　者：张永刚[1,2] 顾溢 马英杰 邵秀梅 李雪[1,2,3] 龚海梅 ZHANG Yong-Gang;GU Yi;MA Ying-Jie;SHAO Xiu-Mei;LI Xue;GONG Hai-Mei(Shanghai Institute of Technical Physics,Chinese Academy of Sciences,Shanghai 200083,China;National Key Laboratory of Infrared Detection Technologies,Shanghai 200083,China;Wuxi Zhongke Deain Sensing Technology Co.,Ltd.,Wuxi 214135,China)

机构地区：[1]中国科学院上海技术物理研究所,上海200083 [2]红外探测全国重点实验室,上海200083 [3]无锡中科德芯感知科技有限公司,江苏无锡214135

出　　处：《红外》2024年第1期1-11,共11页Infrared

基　　金：国家自然科学基金项目(62175250,62075229,62174169,62104238);上海市重点科研计划项目(2019SHZDZX01);上海市优秀学科带头人计划项目(21XD1404200);上海市国际科技合作项目(20520711200)。

摘　　要：人类的探索欲望及数千年来的不断积累促成了20世纪60年代的四大天文发现,而大气层对天文观测的一些根本性限制促使人们在20世纪冲出地球进入太空。在宽广的波段进行天文观测有着极为苛刻的要求,新猜想和模型的提出也要求进行新的验证,这些都促进了观测设备及器件的性能趋于极致。本文旨在对此进行简要的回顾分析并列举一些典型实例,侧重考察其探测波段、主镜或天线的口径、探测仪器及所用器件的类型和性能等,以便进行纵向和横向的比较,温故而思新。The explore desires of human being and the accumulations of thousands year causes four major as-tronomical discoveries in 1960s;whereas some fundamental limitations of our atmosphere on astronomical ob-servation impel us rush out of earth into space.The astronomical observation in such wide of bands arises very critical requirements,new conjectures and models needs new test and verify;all this promote the performance of instruments and devices towards perfection.This article aims to review and analysis the evolution briefly in conjunction with some typical examples,especially their detection bands,diameter of the primary mirror or an-tenna,types of detection instruments and devices as well as related performances.The purpose is for carry on longitudinal and lateral comparisons easier,and gain new ideas by reviewing old.

关 键 词：天文观测 红外 太赫兹 毫米波 射频与微波 

分 类 号：TN2[电子电信—物理电子学]